晴空环境下的地基面天线多场耦合分析及试验

大口径高频段的地基面天线在晴空环境下的热变形对电性能影响明显。针对这一问题,首先     

捷联惯组空间八点减振IMU组合设计CSCD

为了研究捷联惯组空间八点减振IMU组合的力学性能及其在抑制线角耦合方面的作用,采用NX三维建模及ANSYS仿真分析工具对IMU组合的刚度、减振器的线角频率、减振性能方面进行了充分的理论验证。同时,推导出平衡机的调平原理,通过调平使IMU弹性中心与质心重合,然后对惯组进行振动试验,观察其减振性能及三向陀螺角速度输出值。结果表明,经理论分析该IMU组合模态为875.7Hz,具备足够的刚度;减振器线角频率差值在50Hz以上,具有较高的离散度。经试验验证,该IMU组合调平小于0.1mm时,减振效率不低于42%,三向陀螺角速度输出不大于11(°)/s,具有较好的力学环境适应性与极高的角速度输出特性。     

基于正余弦耦合的三轴速率平台控制结构优化

针对三轴速率平台进行三自由度的动态摇摆时出现的平台台体线性漂移问题,提出了一种基于正余弦耦合的三轴速率平台稳定回路控制结构优化方法。当三轴平台进行三自由度摇摆运动时,由于框架间角运动激励的物理耦合和角运动解耦激励的数学耦合,平台台体会产生动态漂移。首先建立三轴平台的角运动输出模型,再根据传递特性将平台基座上的角运动代入到台体伺服控制回路中得到交叉耦合误差项。其次,对比三轴速率陀螺平台和三轴位置陀螺平台在稳定回路控制结构上的异同,分析动态摇摆条件下造成平台台体出现正余弦耦合误差和台体大漂移率误差的形成机理,根据误差源进一步对三轴速率平台的稳定回路控制结构进行了设计优化。最后通过仿真和三自由度转台摇摆试验可见,摇摆过程中不再出现框架角的较大线性漂移,验证了稳定回路结构优化的正确性。     

The Earth’s magnetosphere response to interplanetary medium conditions on January 21–22, 2005 and on December 14–15, 2006

The Earth’s magnetosphere response to interplanetary medium conditions on January 21–22, 2005 and on December 14–15, 2006 has been studied. The analysis of solar wind parameters measured by ACE spacecraft, of geomagnetic indices variations, of geomagnetic field measured by GOES 11, 12 satellites, and of energetic particle fluxes measured by POES 15, 16, 17 satellites was performed together with magnetospheric modeling based in terms of A2000 paraboloid model. We found the similar dynamics of three particle populations (trapped, quasi-trapped, and precipitating) during storms of different intensities developed under different external conditions: the maximal values of particle fluxes and the latitudinal positions of the isotropic boundaries were approximately the same. The main sources caused RC build-up have been determined for both magnetic storms. Global magnetospheric convection controlled by IMF and substorm activity driven magnetic storm on December 14–15, 2006. Extreme solar wind pressure pulse was mainly responsible for RC particle injection and unusual January 21, 2005 magnetic storm development under northward IMF during the main phase.     

内转式进气道/冯·卡门乘波体一体化设计方法

应用特征线理论设计了内转式轴对称基准流场以及外压缩轴对称基准流场,利用激波交线、流线追踪方法等相关技术提出了一种头部进气式的高超声速飞行器内转式进气道/冯·卡门乘波体一体化设计方法,并对生成的一体化构型进行了数值模拟及分析,数值结果验证了该方法的正确性和有效性。该一体化设计方法基本保留了内转式进气道的优良特性,并以高升阻比乘波体为原型构建较高升阻比的一体化构型,从流场耦合的角度出发为减弱机体与进气道之间复杂的波系干扰,实现飞行器内外流的完全耦合进行了探索。     

紧凑式强预冷换热器叉排管束的大涡模拟

采用大涡模拟方法对紧凑式强预冷换热器叉排管束的对流换热问题进行了研究,并运用动力模态分解(DMD)方法对流场的拟序结构及换热统计特性进行了分析.结果表明:在计算工况内(Re≤6000),前排管束的流动结构为有规律的剪切层运动和尾涡脱落.后排管束的流动结构为无规律的小尺度旋涡结构,同时其流场表现出无序性;前排管表面瞬时努...     

运载火箭多体动力学建模与仿真技术研究

针对新一代运载火箭结构动力学与控制系统耦合强烈、严重影响火箭的飞行稳定问题,提出一种基于多体动力学虚拟样机建模与仿真的方法,有效解决运载火箭姿态动力学模型地面难以验证的困难.首先阐述了在运载火箭姿态动力学分析中应用多体虚拟样机的基本思路;然后对多体动力学模型与传统火箭姿态动力学模型在建模原理上的差异进行分析,指出引入多...     

From the Solar Wind to the Magnetospheric Substorm

This paper gives a brief outline of the progression from the first substorm model developed in Ref.[4] and[8] based on Kennel's ideas[3], to the present views about the mechanism by which solar wind kinetic energy is converted to electromagnetic energy at the Bow Shock and by which this energy is transferred to the magnetosphere in the form of current; about the transformation of the energy of this current to gas kinetic energy of convecting plasma tubes, and, finally, the back transformation of gas kinetic energy to electromagnetic energy in secondary magnetospheric MHD generators. The questions of the formation of the magnetospheric convection system, the nature of substorm break-up, and of the matching of currents in the magnetosphere-ionosphere system are discussed.      

介质谐振腔滤波器的设计

论述了介质谐振腔滤波器的设计与制造;给出了计算谐振频率的经典计算公式和制作实例的照片及响应曲线;介绍了设计谐振腔之间耦合系数的方法和相关曲线,并综述了新的发展动向。